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20002026
most citedObservations of Disequilibrium CO Chemistry in the Coldest Brown Dwarfs

94 citations · 624 across the 18 of their papers we have counts for

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astro-ph.EP2026

Water Cloud and Chemical Modulations in the Coldest Brown Dwarf

Brittany E. Miles, James Mang, Caroline V. Morley +24

We present high signal-to-noise, medium resolution (R ~ 1000), time-series JWST/NIRSpec spectra of WISE 0855 (265K), the coldest known brown dwarf. Medium resolution, time-series s…

astro-ph.EP2020★ 94 cited

Observations of Disequilibrium CO Chemistry in the Coldest Brown Dwarfs

Brittany E. Miles, Andrew J. I. Skemer, Caroline V. Morley +10

Cold brown dwarfs are excellent analogs of widely separated, gas giant exoplanets, and provide insight into the potential atmospheric chemistry and physics we may encounter in obje…

astro-ph.EP2019★ 44 cited

First ALMA Millimeter Wavelength Maps of Jupiter, with a Multi-Wavelength Study of Convection

Imke de Pater, R. J. Sault, Chris Moeckel +15

We obtained the first maps of Jupiter at 1-3 mm wavelength with the Atacama Large Millimeter/Submillimeter Array (ALMA) on 3-5 January 2017, just days after an energetic eruption a…

astro-ph.EP2019★ 21 cited

Cassini Composite Infrared Spectrometer (CIRS) Observations of Titan 2004--2017

Conor A. Nixon, Todd M. Ansty, Nicholas A. Lombardo +16

From 2004 to 2017, the Cassini spacecraft orbited Saturn, completing 127 close flybys of its largest moon, Titan. Cassini's Composite Infrared Spectrometer (CIRS), one of 12 instru…

astro-ph.EP2018★ 53 cited

A Hexagon in Saturn's Northern Stratosphere Surrounding the Emerging Summertime Polar Vortex

L. N. Fletcher, G. S. Orton, J. A. Sinclair +13

Saturn's polar stratosphere exhibits the seasonal growth and dissipation of broad, warm, vortices poleward of latitude, which are strongest in the summer and absent…

astro-ph.EP2018★ 40 cited

The Gas Composition and Deep Cloud Structure of Jupiter's Great Red Spot

Gordon L. Bjoraker, Michael H. Wong, Imke de Pater +3

We have obtained high-resolution spectra of Jupiter's Great Red Spot (GRS) between 4.6 and 5.4 microns using telescopes on Mauna Kea in order to derive gas abundances and to constr…